... C'est avec beaucoup d'?motion que je me souviens des nombreuses rencontres avec M.M. Molodensky, que nous avions pris l'habitude d'appeler affectueusement, parmi quelques intimes, Misha, et qui nous a toujours fait le privil?ge de l'appr?cier. ... Ce f?t le d?but d'une longue collaboration que nous avons poursuivie a l'occasion de plusieurs s?jours qu'il p?t r?aliser en France bien plus tard, gr?ce a des actions d'ailleurs pas toujours tr?s orthodoxes. ... Il nous manque. ...
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... Impact on source motion in Galactic coordinate system is given by Kovalevsky (2003), Malkin (2011) l cos b = -A sin l, b = -A cos l sin b, where A = R0 02 /c is the galactocentric acceleration called hereafter the GA constant. ... We just have to return to the traditional many-centuries-old astrometric practice of modelling the position of a celestial object as a linear trend with two parameters: the position at the initial (conventional) epoch and the apparent (proper) motion. ... 2011). ...
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